Why Is Gravitational Acceleration Least at the Equator and Maximum at the Poles?

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Homework Help Overview

The discussion centers around the variation of gravitational acceleration on Earth, specifically why it is least at the equator and maximum at the poles. Participants explore the effects of Earth's rotation and its shape on gravitational forces.

Discussion Character

  • Exploratory, Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants discuss the role of Earth's oblateness and centrifugal force in gravitational acceleration differences. Questions arise about the relationship between centripetal acceleration and linear velocity at different latitudes.

Discussion Status

The discussion is active, with various interpretations being explored regarding the factors influencing gravitational acceleration. Some participants offer insights into the physics of rotation and its effects, while others seek clarification on specific points raised.

Contextual Notes

There is an emphasis on the effective gravitational acceleration, which includes corrections for Earth's non-spherical shape and rotation. Some participants note the complexity of the question and the need for careful consideration of the forces at play.

Milind_shyani
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The gravitational acceleration at the equator is the least and at the pole is the maximum due to the rotation of the Earth on its axis.Why?
 
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The Earth is not precisely spherical, it is flattened at the poles because of the Earth's rotation. This is simply because of the centrifugal force, objects at the equator have the greatest distance from the axis of rotation so are 'flung outwards' more than at the poles. So at the poles you are closer to the center of the Earth and experience a greater gravitational acceleration.
 
It should be borne in mind that "g" is generally meant to mean "effective gravitational acceleration" and includes the effects of a rotating Earth (which predicts a lower g at equator than by the poles), the deviatioric correction due to the non-spherical form of the Earth, as the two main correctional effects.
 
Galileo is right - the oblateness of the Earth is the biggest factor in the difference in gravitational attraction.

However, the way the question is worded, I think it's addressing centripetal acceleration. Which point will have a larger linear velocity due to the rotation of the Earth: a point on the equator or a point on one of the poles?

Both the oblateness of the Earth and centripetal force contribute to reducing the net force, and the resulting acceleration, at the equator (with oblateness having nearly twice as much affect).
 
I never said that Galileo was wrong..
 
arildno said:
I never said that Galileo was wrong..
I did (or at least said that his answer didn't answer the question that was asked).

I didn't comment on your answer because I didn't understand it. :smile:
 
To the OP -- just think about what happens as you spin the Earth faster and faster...what force is acting on the person at the equator that is different from the person at the pole? Quiz question -- how fast to you have to spin the Earth to spit off the person at the equator?
 
Think of a girl on a merry-go-round. She will move at a larger speed when she is further away from the center, since the outer regions cover a larger distance in the same time. If the merry-go-round would spin faster and faster the girl would have to hold on for dear life or she would be flung off. She would conclude that some force is pulling her outwards from the center. This force we call the centrifugal force, it is not a real force. It results from her inertia - she wants to keep on moving in a straight line and have to hold on or press up against something in order to keep on the merry-go-round. The same happens with an object on the earth. The further it is away from the rotation axis of the Earth the larger the centrifugal force it experiences. This leads to a decrease in the weight of the object - it wants to fly off the earth. Since the weight is related to the gravitational acceleration and mass (which stays the same under all circumstances) we conclude that gravity was somehow reduced by this effect.
 
The effect of 'centrifugal' acceleration can be quanitfied by;
[tex]g_{a} = g - r\omega^2\cos^2\theta[/tex]
where [itex]g_{a}[/itex] is the apparent force of gravity and [itex]\theta[/itex] is latitude. This assumes the Earth is spherical, but is a good approximation for a non-spherical earth.
 

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